Collinder 196

(MWSC 1552; OCL 721; ESO 432 07)

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0.23 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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Collinder 196 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.12 kpc) differs significantly from the median photometric distance (~1.05 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 131.308 -31.737 0.32 -4.69 3.023 –
Just et al. 2023 131.251 -31.622 – – – –
Bica et al. 2019 131.28 -31.647 – – – –
Kharchenko et al. 2016 131.251 -31.622 – – – –
Kharchenko et al. 2013 131.257 -31.625 – -3.94 1.06 –
Bukowiecki et al. 2011 131.308 -31.6 – – – –
Dias et al. 2002 131.25 -31.633 – -16.6 8.92 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.05 0.655 – 1820 – 112 – –
Just et al. 2023 – – – 1820 – 178 – –
Kharchenko et al. 2016 1.39 0.78 – 1820 – – – –
Kharchenko et al. 2013 1.39 0.78 – 1820 – – – –
Bukowiecki et al. 2012 – – – – – 47 – –
Bukowiecki et al. 2011 0.71(1) 0.53 – 79 – – – –
Dias et al. 2002 0.66 0.53 – 79 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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